The Keck Baryonic Structure Survey: using foreground/background galaxy pairs to trace the structure and kinematics of circumgalactic neutral hydrogen at z ∼ 2.

We present new measurements of the spatial distribution and kinematics of neutral hydrogen in the circumgalactic and intergalactic medium surrounding star-forming galaxies at z ∼ 2. Using the spectra of ≃3000 galaxies with redshifts 〈 z 〉 = 2.3 ± 0.4 from the Keck Baryonic Structure Survey, we assemble a sample of more than 200 000 distinct foreground-background pairs with projected angular separations of 3–500 arcsec and spectroscopic redshifts, with 〈 z _fg〉 = 2.23 and 〈 z _bg〉 = 2.57 (foreground, background redshifts, respectively.) The ensemble of sightlines and foreground galaxies is used to construct a 2D map of the mean excess |$\rm{H\,{\small I}}$| |$\rm Ly\,\alpha$| optical depth relative to the intergalactic mean as a function of projected galactocentric distance (20 ≲ D _tran/pkpc ≲ 4000) and line-of-sight velocity. We obtain accurate galaxy systemic redshifts, providing significant information on the line-of-sight kinematics of |$\rm{H\,{\small I}}$| gas as a function of projected distance D _tran. We compare the map with cosmological zoom-in simulation, finding qualitative agreement between them. A simple two-component (accretion, outflow) analytical model generally reproduces the observed line-of-sight kinematics and projected spatial distribution of |$\rm{H\,{\small I}}$|⁠. The best-fitting model suggests that galaxy-scale outflows with initial velocity v _out ≃ 600 km s ^{|$^{-1}\,$|} dominate the kinematics of circumgalactic |$\rm{H\,{\small I}}$| out to D _tran ≃ 50 kpc, while |$\rm{H\,{\small I}}$| at D _tran ≳ 100 kpc is dominated by infall with characteristic v _in ≲ circular velocity. Over the impact parameter range 80 ≲ D _tran/pkpc ≲ 200, the |$\rm{H\,{\small I}}$| line-of-sight velocity range reaches a minimum, with a corresponding flattening in the rest-frame |$\rm Ly\,\alpha$| equivalent width. These observations can be naturally explained as the transition between outflow-dominated and accretion-dominated flows. Beyond D _tran ≃ 300 pkpc (∼1 cMpc), the line-of-sight kinematics are dominated by Hubble expansion. [ABSTRACT FROM AUTHOR]